1 00:00:02,040 --> 00:00:06,720 Speaker 1: Welcome to brain stuff from how stuff works, Hey, brain 2 00:00:06,800 --> 00:00:10,280 Speaker 1: stuff loring vogel bomb here. Nuclear pasta might sound like 3 00:00:10,360 --> 00:00:12,639 Speaker 1: a fancy concoction cooked up by a chef working in 4 00:00:12,720 --> 00:00:17,000 Speaker 1: molecular astronomy, but it's actually light years away, literally from 5 00:00:17,079 --> 00:00:20,200 Speaker 1: the spaghetti you'd find in the kitchen. This weird kind 6 00:00:20,239 --> 00:00:23,400 Speaker 1: of noodle is needed below the crust of neutron stars, 7 00:00:23,720 --> 00:00:26,800 Speaker 1: and in a new study, a powerful computer simulation has 8 00:00:26,880 --> 00:00:30,080 Speaker 1: taken a stab at manipulating this stellar noodle and found 9 00:00:30,200 --> 00:00:34,239 Speaker 1: that it's the strongest material in the cosmos. So how 10 00:00:34,320 --> 00:00:38,280 Speaker 1: did this nuclear pasta become the super Macaroni of the universe. Well, 11 00:00:38,360 --> 00:00:41,720 Speaker 1: it's because it's created inside neutron stars, which act like 12 00:00:41,880 --> 00:00:46,320 Speaker 1: extreme pressure cookers. Neutron stars are these stellar corpses of 13 00:00:46,479 --> 00:00:49,040 Speaker 1: massive stars that have run out of fuel and exploded 14 00:00:49,080 --> 00:00:52,920 Speaker 1: as supernova. These tiny, fast spinning objects are only a 15 00:00:53,000 --> 00:00:55,440 Speaker 1: dozen or so miles wide and yet pack in the 16 00:00:55,720 --> 00:00:59,200 Speaker 1: entire mass of our Sun. They're so dense that only 17 00:00:59,280 --> 00:01:02,080 Speaker 1: a teaspoon full of neutron star matter weighs as much 18 00:01:02,120 --> 00:01:05,280 Speaker 1: as a mountain on Earth. Neutron stars are therefore not 19 00:01:05,440 --> 00:01:10,040 Speaker 1: composed of normal matter, but rather what astrophysicists call degenerate matter. 20 00:01:10,520 --> 00:01:13,039 Speaker 1: It's not an insult. It's just the term for extremely 21 00:01:13,120 --> 00:01:18,080 Speaker 1: compact neutrons that are crushed together under incredibly powerful gravitational forces. 22 00:01:19,080 --> 00:01:21,880 Speaker 1: A neutron star is extreme gravity makes its outer layers 23 00:01:22,000 --> 00:01:24,600 Speaker 1: freeze solid as a crust with a liquid core below. 24 00:01:25,360 --> 00:01:29,000 Speaker 1: Underneath the crust, powerful forces royal between the neutrons and 25 00:01:29,080 --> 00:01:32,640 Speaker 1: protons inside the neutron stars matter, causing the material to 26 00:01:32,760 --> 00:01:36,640 Speaker 1: take on some surprising shapes like long cylinders and flat planes. 27 00:01:37,440 --> 00:01:41,280 Speaker 1: Astrophysicists refer to these shapes as things like lasagna, spaghetti, 28 00:01:41,480 --> 00:01:46,080 Speaker 1: and nioki, and collectively as nuclear pasta because astro physicists 29 00:01:46,120 --> 00:01:49,360 Speaker 1: get to make their own fun. Understanding how this nuclear 30 00:01:49,440 --> 00:01:53,600 Speaker 1: pasta works is a key concern. A researcher Matthew Kaplan, 31 00:01:53,880 --> 00:01:57,440 Speaker 1: a postdoctoral research fellow at McGill University, set in a statement, 32 00:01:57,800 --> 00:02:00,559 Speaker 1: the strength of the neutron star crust, especially the bottom 33 00:02:00,560 --> 00:02:03,080 Speaker 1: of the crust, is relevant to a large number of 34 00:02:03,160 --> 00:02:07,360 Speaker 1: astrophysics problems, but isn't well understood. Their outer layers the 35 00:02:07,400 --> 00:02:10,079 Speaker 1: part we actually observe, So we need to understand that 36 00:02:10,200 --> 00:02:14,919 Speaker 1: in order to interpret astronomical observations of these stars. To 37 00:02:15,000 --> 00:02:17,919 Speaker 1: get a better understanding of this noodly mess, Kaplan and 38 00:02:17,960 --> 00:02:21,240 Speaker 1: his team created the most complex computer simulation ever carried 39 00:02:21,280 --> 00:02:24,360 Speaker 1: out on neutron star crusts to understand how they warp 40 00:02:24,560 --> 00:02:27,880 Speaker 1: and break. It turns out that nuclear pasta is way 41 00:02:27,960 --> 00:02:31,959 Speaker 1: beyond al Dente. It's the strongest known material in the universe. 42 00:02:32,760 --> 00:02:36,760 Speaker 1: This is especially important as physicists can now measure gravitational waves, 43 00:02:37,200 --> 00:02:40,480 Speaker 1: the ripples in space time caused by massive cosmic objects 44 00:02:40,600 --> 00:02:44,040 Speaker 1: like neutron stars and black holes spinning, colliding, and merging. 45 00:02:44,760 --> 00:02:47,720 Speaker 1: The crust of neutron stars is therefore very important for 46 00:02:47,800 --> 00:02:51,560 Speaker 1: science to understand. In fact, low neutron stars may produce 47 00:02:51,639 --> 00:02:55,160 Speaker 1: their own weak gravitational waves by creating rigid mountains in 48 00:02:55,240 --> 00:02:59,079 Speaker 1: their crests. As neutron stars spin, these mountains would disturb 49 00:02:59,160 --> 00:03:02,320 Speaker 1: space time like a propeller cutting through a calm lake surface, 50 00:03:02,760 --> 00:03:05,760 Speaker 1: generating a constant source of gravitational waves that we may 51 00:03:05,840 --> 00:03:09,120 Speaker 1: be able to detect in the future. Kaplan said, a 52 00:03:09,200 --> 00:03:12,320 Speaker 1: lot of interesting physics is going on here under extreme conditions, 53 00:03:12,639 --> 00:03:15,359 Speaker 1: and so understanding the physical properties of a neutron star 54 00:03:15,720 --> 00:03:18,000 Speaker 1: is a way for scientists to test their theories and 55 00:03:18,120 --> 00:03:21,800 Speaker 1: models With this result, many problems need to be revisited. 56 00:03:22,360 --> 00:03:24,239 Speaker 1: How large a mountain can you build on a neutron 57 00:03:24,320 --> 00:03:26,959 Speaker 1: star before the crust breaks and it collapses, what will 58 00:03:27,000 --> 00:03:30,760 Speaker 1: it look like, and most importantly, how can astronomers observe it? 59 00:03:31,960 --> 00:03:34,320 Speaker 1: So the next time you're boiling your penny, take a 60 00:03:34,360 --> 00:03:36,800 Speaker 1: minute to ponder the mountains of nuclear pasta that could 61 00:03:36,840 --> 00:03:39,320 Speaker 1: feed us a lot about the nature of neutron stars. 62 00:03:44,480 --> 00:03:47,040 Speaker 1: Today's episode was written by Ian O'Neill and produced by 63 00:03:47,120 --> 00:03:49,440 Speaker 1: Tyler Clang. For more on this end lots of other 64 00:03:49,520 --> 00:03:52,839 Speaker 1: Noodley topics, visit our home planet, how Stuff Works dot com.